Search for γ-ray emission from superluminous supernovae with the Fermi-LAT

被引：17
|
作者：
Renault-Tinacci, N. [1 ,2 ,3 ]
Kotera, K. [1 ,2 ,3 ]
Neronov, A. [4 ]
Ando, S. [5 ]
机构：
[1] Univ Paris 06, Sorbonne Univ, UPMC, 98bis Bd Arago, F-75014 Paris, France
[2] Inst Astrophys Paris, CNRS, UMR 7095, 98bis Bd Arago, F-75014 Paris, France
[3] Univ Paris Diderot, CNRS, Lab AIM Paris Saclay, CEA,DSM,IRFU, F-91191 Gif Sur Yvette, France
[4] Univ Geneva, Astron Dept, Ch Ecogia 16, CH-1290 Versoix, Switzerland
[5] Univ Amsterdam, GRAPPA Inst, NL-1098 XH Amsterdam, Netherlands
来源：
ASTRONOMY & ASTROPHYSICS | 2018年 / 611卷
关键词：
gamma rays: general; supernovae: general; CENTRAL COMPACT OBJECT; LARGE-AREA TELESCOPE; PULSAR WIND NEBULAE; MAGNETIC-FIELD; SPECTRAL EVOLUTION; SHOCK-BREAKOUT; LIGHT CURVES; PROBE; STAR; ACCELERATION;
D O I：
10.1051/0004-6361/201730741
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the first individual and stacking systematic search for gamma-ray emission in the GeV band in the directions of 45 superluminous supernovae (SLSNe) with the Fermi Large Area Telescope (LAT). No excess of gamma-rays from the SLSN positions was found. We report gamma-ray luminosity upper limits and discuss the implication of these results on the origin of SLSNe and, in particular, the scenario of central compact object-aided SNe. From the stacking search, we derived an upper limit at 95% confidence level to the gamma-ray luminosity (above 600 MeV) L-gamma < 9.1 x 10(41) erg s(-1) for an assumed E-2 photon spectrum for our full SLSN sample. We conclude that the rate of the neutron stars born with millisecond rotation periods P <= 2 ms and B similar to 10(12-13) G must be lower than the rate of the observed SLSNe. The luminosity limits obtained on individual sources are also constraining: in particular, SN2013fc, CSS140222, SN2010kd, and PTF12dam can only be born with millisecond periods if B <= 10(13) G.
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页数：11
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